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BN天体

贝克林-诺伊格鲍尔天体
Becklin-Neugebauer Object
觀測資料
曆元 J2000.0
星座 猎户座
星官
赤經 05h 35m 14.113s[1]
赤緯 -05° 22′ 22.73″[1]
視星等(V)
特性
光谱分类B[2]
天体测定
距离~1500[3] ly
詳細資料
質量7[2] M
其他命名
V2254 Ori, 2MASS J05351411-0522227
參考資料庫
SIMBAD资料

贝克林-诺伊格鲍尔天体(简称BN天体,英語:Becklin-Neugebauer Object)是獵戶座分子雲團中一个仅能通过红外观测到的天体。它于1967年由埃里克·贝克林(Eric Becklin)和格里·诺伊格鲍尔(Gerry Neugebauer)发现。

BN天体被认为是一颗中等质量的原恒星,约为15太阳质量。它还是除太阳外在10微米波长以下最为明亮的天体。[4]

参考资料

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  1. ^ 1.0 1.1 [ NAME BN Object] 请检查|url=值 (帮助). SIMBAD. 斯特拉斯堡天文資料中心. [2016-11-16]. 
  2. ^ 2.0 2.1 Tan, Jonathan C. The Becklin-Neugebauer Object as a Runaway B Star, Ejected 4000 Years Ago from the θ1 Orionis C System (PDF). Astrophysical Journal. 20 May 2004, 607: 47–50 [2016-08-21]. Bibcode:2004ApJ...607L..47T. arXiv:astro-ph/0401552可免费查阅. doi:10.1086/421721. 
  3. ^ The Becklin-Neugebauer Object: Circumstellar Disk Cradles Young Massive Star. Adaptiveoptics.org. 31 August 2005 [2016-08-21]. (原始内容存档于2016-03-03). 
  4. ^ Becklin-Neugebauer Object. The Internet Encyclopedia of Science. [2010-03-06]. (原始内容存档于2010-05-30). 

外部链接

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BN天体
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